Table 3
Observed flux (F) and intrinsic luminosity (L) of IC 4329A over various energy bands.
| F | L | |
|---|---|---|
| Energy range | (10−11 erg cm−2 s−1) | (1044 erg s−1) |
| Hard X-ray (2–10 keV) | 11.0 (2003) | 0.7 (2003) |
| 14.2 (2017) | 0.9 (2017) | |
| Soft X-ray (0.2–2 keV) | 3.0 (2003) | 1.4 (2003) |
| 3.7 (2017) | 1.6 (2017) | |
| EUV (100–1000 Å) | 8 × 10−7 | 5.8 |
| UV (1000–4000 Å) | 0.2 | 4.5 |
| Optical (4000–7000 Å) | 2.2 | 1.0 |
| Near-IR (0.7–3 μm) | 23.5 | 1.5 |
| Mid-IR (3–40 μm) | 64.6 | 3.9 |
| Far-IR (40–500 μm) | 10.8 | 0.7 |
| 1–1000 Ryd | 16.9 (2003) | 8.5 (2003) |
| 21.6 (2017) | 9.1 (2017) | |
| Bolometric (10−6–103 keV) | 152.0 (2003) | 24.5 (2003) |
| 164.9 (2017) | 26.4 (2017) |
Notes. The values correspond to the SEDs shown in Fig. 3. The continuum modelling is described in Sect. 3 (Table 2). The observed fluxes (F) include the effects of all the reddening and absorption components. The host galaxy optical and UV emission, and the AGN BLR and NLR emission, are excluded from the reported fluxes and luminosities. The IR fluxes and luminosities include all the dust emission components.
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